Continued Study of Highly Siderophile Element Characteristics of Apollo 17 Impact Melt Breccias

Details Continued Study of Highly Siderophile Element Characteristics of Apollo 17 Impact Melt Breccias Continued Study of Highly Siderophile Element Characteristics of Apollo 17 Impact Melt Breccias

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.1413g&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.1413

Physics

Scientific paper

187Os/188Os and Ru, Pd, Re, Ir, Os, and Pt abundances for impact melt
breccias 72435, 72535, and 73235 are reported. Results were similar to
measured poikilitic Apollo 17 rocks consistent with the interpretation
of one single Serenitatis impactor.

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